Welcome to the standard form calculator, where we'll learn how to write a number in standard form. "What is the standard form?" Well, we'll get to the standard form definition soon enough. But let's just say that standard form in math and physics (quite often called scientific notation) is a neat way of dealing with values that are either very large or very small. It's quite troublesome to write all the zeros of a number in every line of our calculations. Preferably, we can use standard form exponents and write the same thing with just a few symbols. That's why we made this standard form converter - to help you with just that.

Warning: There is a possibility that you've come across this standard form calculator in search of different ways of writing a quadratic equation. In that case, check out our quadratic formula calculator, but be sure to come back to us whenever you get the chance!

Now, back to the question of the hour, "What does standard form mean?"

What is the standard form?

As we've already said above, writing numbers in standard form is useful whenever we have some values that are either very large, or very small. Formally, the standard form definition is

a = b * 10ⁿ,


  • a is the number we want to convert to standard form;
  • b is a value between 1 and 10 (including 1 but excluding 10); and
  • n is some integer (possibly negative).

So what does standard form mean? In essence, it tells you to take the significant figures that tell you (with some precision) what the value is, and then separately write the order of magnitude using the standard form exponents. To give you an example of how we use the standard form definition in real life, recall the stimulus check given to American citizens by the authorities and how much money it involved. It's much easier to write (and read) that it was a $2 trillion, rather than a $2,000,000,000,000 package, wouldn't you say?

Alright, let's now take a look at how we convert to standard form.

What does standard form mean?

Before we give some examples of writing numbers in standard form in physics or chemistry, let's recall from the above section the standard form math formula:

a = b * 10ⁿ.

We said that the number b should be between 1 and 10. This means that, for example, 1.36 * 10⁷ or 9.81 * 10⁻²³ are in standard form, but 13.1 * 10¹² isn't because 13.1 is bigger than 10. We could, however, convert it to standard form by saying that

13.1 * 10¹² = 1.31 * 10¹³.

What we've done above is basically move the point, ., that separates the digits of the number by one place, which is equivalent to 10 to the power of one. And that is exactly what the standard form exponents are for.

If we take a number, say, 12,345.6789, and multiply it by 10, we'll get

12,345.6789 * 10¹ = 123,456.789.

In other words, we move the point one place to the right. If we do it again, we'll get

(12,345.6789 * 10¹) * 10¹ = 12,345.6789 * 10² = 1,234,567.89,

which is the number we had initially but with the point two places to the right. This movement by 2 is shown by the power in the standard form exponents.

Conversely, if we divide the initial number by 10, which is equal to multiplying it by 1/10 = 10⁻¹, we'll get

12,345.6789 * 10⁻¹ = 1,234.56789,

which is the value we had but with the point one place to the left.

To sum up, in the standard form math formula

a = b * 10ⁿ,

the absolute value of the standard form exponents n tell us how many places we have to move the point, and the sign of n indicates if it should be to the right (for n positive) or the left (for n negative). Therefore, when we convert to standard form, it's all about choosing the power of 10 in such a way so that the b in the formula is between 1 and 10.

Alright, after all this time learning the theory, it's finally time we saw some standard form examples, wouldn't you say?

Standard form examples

Now that we've seen how to write a number in standard form, it's time to convince you that it's a useful thing to do. Of course, we know that you're most probably learning all of this for the pure pleasure of grasping yet another part of theoretical mathematics, but it doesn't hurt to take a look at physics or chemistry from time to time. You know, those two minor branches of mathematics.

In the first section, we mentioned that the standard form converter is most useful when we're dealing with very large or very small numbers. So, why don't we take one object from each side of the spectrum: a planet and an atom.

The mass of the Earth is, approximately,

5,972,000,000,000,000,000,000,000 kg

and its circumference is

40,075 km.

Don't ask us how they found the mass of the Earth, there aren't any scale big enough to weigh the entire planet. As for the circumference, talk to Eratosthenes.

Anyway, if scientists had to write all of those zeros every time they calculated something about our planet, they'd waste ages! It's much easier to recall how to write a number in standard form and say that the mass of Earth is, in fact,

5.972 * 10²⁴ kg

and the circumference is... actually, the 40,075 km doesn't look that bad, does it? Well, we could change it into 4.0075 * 10⁴ km, but is it better that way? If we needed to change it to millimeters, then maybe it'd be a better idea, but the kilometer form seems perfectly usable.

There is a valuable lesson here: writing numbers in standard form is not always the way to go. It's all about simplicity of notation, but, at the end of the day, it pretty much boils down to a matter of personal preference (or your teacher's if you're writing a test).

Back to the standard form examples, the mass of a helium atom is (approximately)

0.0000000000000000000000000066423 kg

and its radius is

0.00000000014 m.

Now, this looks even worse than the previous example, it doesn't have the commas in between! Thankfully, there are tools - like our standard form calculator - to make our lives easier. So, what is the standard form of the above numbers?

6.6423 * 10⁻²⁷ kg and

1.4 * 10⁻¹⁰ m.

Arguably, there is now no question that writing the numbers in standard form was a good idea.

Example: using the standard form calculator

Suppose that you've taken up astronomy recently, and would like to know the gravitational force acting between the Earth and the Moon. For the calculations, we need the masses of the two objects (denote the Earth's by M₁ and the Moon's by M₂) and the distance between them (denoted by R). We have

M₁ = 5,972,000,000,000,000,000,000,000 kg,

M₂ = 73,480,000,000,000,000,000,000 kg, and

R = 384,400,000 m.

If you look at our gravitational force calculator, you'll find that we'll be using the formula

F = G * M₁ * M₂ / R²,


  • G is the gravitational constant, G = 0.00000000006674 N*m²/kg².

All in all, the gravitational force is

F = 0.00000000006674 N*m²/kg² * 5,972,000,000,000,000,000,000,000 kg * 73,480,000,000,000,000,000,000 kg / (384,400,000 m)².

Um... maybe we should reconsider that and try our standard form calculator. What do you say?

Let's input the four above numbers into our standard form converter. It will tell us that

M₁ = 5.972 * 10²⁴ kg,

M₂ = 7.348 * 10²² kg,

R = 3.844 * 10⁸ m, and

G = 6.674 * 10⁻¹¹ N*m²/kg².

All in all, we can rewrite our formula as

F = 6.674 * 10⁻¹¹ N*m²/kg² * 5.972 * 10²⁴ kg * 7.348 * 10²² kg / (3.844 * 10⁸ m)².

Now, this is more like it! We don't know about you, but for us short is beautiful, in mathematics at least.

But there's more! We have multiplication and division in the formula, and the standard form exponents make these two operations very easy to calculate. By the well-known, well-remembered, and totally not forgotten the moment the test was over formulas, multiplying two powers with the same base is the same as adding the exponents, while dividing corresponds to subtracting them. In other words, if we separate the 10's to some powers from the other numbers, we'll get

F = (6.674 * 5.972 * 7.348 / 3.844²) * (10⁻¹¹ * 10²⁴ * 10²² / (10⁸)²) N,

which is

F = (6.674 * 5.972 * 7.348 / 3.844²) * 10⁻¹¹⁺²⁴⁺²²⁻¹⁶ N.

Now it's just a few good old calculations to get:

F ≈ 19.82 * 10¹⁹ N.

We've spent quite some time together with the standard form calculator, enough to know that we can't leave the answer like this. We haven't learned how to write a number in standard form for nothing.

F ≈ 1.982 * 10²⁰ N.

Now that we know with what force the Earth attracts the Moon, maybe we could do something similar to get the attraction between you and your crush?

Maciej Kowalski, PhD candidate